Star Algebra Spectroscopy
Author(s) -
Leonardo Rastelli,
Ashoke Sen,
Barton Zwiebach
Publication year - 2002
Publication title -
journal of high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.998
H-Index - 261
eISSN - 1126-6708
pISSN - 1029-8479
DOI - 10.1088/1126-6708/2002/03/029
Subject(s) - eigenvalues and eigenvectors , degenerate energy levels , mathematics , spectrum (functional analysis) , wedge (geometry) , pure mathematics , vertex (graph theory) , physics , combinatorics , quantum mechanics , geometry , graph
The spectrum of the infinite dimensional Neumann matrices M^{11}, M^{12} andM^{21} in the oscillator construction of the three-string vertex determines keyproperties of the star product and of wedge and sliver states. We study thespectrum of eigenvalues and eigenvectors of these matrices using the derivationK_1 = L_1 + L_{-1} of the star algebra, which defines a simple infinite matrixcommuting with the Neumann matrices. By an exact calculation of the spectrum ofK_1, and by consideration of an operator generating wedge states, we are ableto find analytic expressions for the eigenvalues and eigenvectors of theNeumann matrices and for the spectral density. The spectrum of M^{11} iscontinuous in the range [-1/3, 0) with degenerate twist even and twist oddeigenvectors for every eigenvalue except for -1/3.Comment: LaTeX, 30 pages, 2 figure
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